Gyroscopic motion and aberration in stationary fields

Details Gyroscopic motion and aberration in stationary fields Gyroscopic motion and aberration in stationary fields

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978phrvd..17..972g&link_type=abstract

Physical Review D (Particles and Fields), Volume 17, Issue 4, 15 February 1978, pp.972-975

Physics

1

Scientific paper

A method developed earlier for calculating the combined gyroscopic
precession and starlight aberration is extended to stationary metrics
and nongeodesic motion. Results include periodic and secular terms. The
secular terms for circular motion agree with presently accepted values.

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